Down |
2. | The region surrounding the earth or another astronomical body in which its magnetic field is the predominant effective magnetic field |
4. | A unit of length equal to about 149,597,870.7 kilometers |
5. | A meteor that survives its passage through the earth's atmosphere such that part of it strikes the ground |
6. | A massive, gravitationally bound system that consists of stars and stellar remnants |
7. | The theory that the universe originated sometime between 10 billion and 20 billion years ago from the cataclysmic explosion of a small volume of matter at extremely high density and temperature |
8. | Shifting Patterns of coloured light that appear in the night sky in northern latitudes |
9. | A region of space having a gravitational field so intense that no matter or radiation can escape |
10. | Temporary phenomena on the photosphere of the Sun that appear visibly as dark spots compared to surrounding regions |
11. | An increase (or decrease) in the frequency of sound, light, or other waves as the source and observer move toward (or away from) each other |
12. | A group of stars forming a pattern that is traditionally named after its apparent form or identified with a mythological figure |
15. | The direction opposite to the movement of something else |
18. | A massive and extremely remote celestial object, emitting exceptionally large amounts of energy, and typically having a starlike image in a telescope |
23. | A planet whose orbit lies within the asteroid belt |
24. | Earth-Centered model of the solar system |
25. | The effect whereby the position or direction of an object appears to differ when viewed from different positions |
26. | The luminous envelope of a star from which its light and heat radiate |
27. | The tracing and measurement of a series or network of triangles in order to determine the distances and relative positions of points spread over a territory or region |
29. | The intrinsic brightness of a celestial object |
30. | The process or result of joining two or more things together to form a single entity |
31. | The rarefied gaseous envelope of the sun and other stars |
34. | Move in a circle on a central axis |
36. | An angular measurement in a spherical coordinate system |